Properties of H α -selected star-forming galaxies from z ~ 0.8 to now

Bibcode
2005RMxAC..24..268P
Pascual, S.; Villar, V.; Gallego, J.; Zamorano, J.; Pelló, R.; Díaz, C.; Aragón-Salamanca, A.
Bibliographical reference

II International GTC Workshop: Science with GTC 1st-light Instruments and the LMT (Eds. A. M. Hidalgo-Gámez, J. J. González, J. M. Rodríguez Espinosa, and S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 24, pp. 268-269 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
12
2005
Number of authors
7
IAC number of authors
0
Citations
1
Refereed citations
1
Description
We present a long-term project to study the characteristics and evolution of current star-forming galaxies at different redshifts. Our results support the idea that the higher Star Formation Density measured at redshift z=0.24 is due to an increase of the density of bursting galaxies and not to an intrinsic change on overall galaxy properties.
Type
Non-refereed
Galaxies
Star formation

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